We use bilby_pipe and Bilby [1]} to simulate 128 injections using IMRPhenomPv2 [2]}, [3]} sampled at 2048 Hz with 4-second observing time in a three detector network with AdLIGO Hanford, AdLIGO Livingston and AdVirgo at design sensitivity [4]}. We choose uniform priors on chirp mass \(\mathcal {M} \sim \mathcal {U} [[25, 35]]{\text{M}_{\odot }}\)  and asymmetric mass ratio \(q \sim \mathcal {U}[0.125, 1.0]\) , a prior on luminosity distance that is uniform in co-moving volume on \([[100, 2000]]\,{\text{Mpc}}\) , a uniform prior for the reference time at the geocentre with width 0.2 and the remaining priors are set to the defaults for precessing binary black holes in Bilby [5]}, see app:priors for a complete list.
